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The Lower Gila Region, Arizona
DEPARTMENT OF THE INTERIOR HUBERT WORK, Secretary UNITED STATES GEOLOGICAL SURVEY GEORGE OTIS SMITH, Director Water-Supply Paper 498 THE LOWER GILA REGION, ARIZONA A GEOGBAPHIC, GEOLOGIC, AND HTDBOLOGIC BECONNAISSANCE WITH A GUIDE TO DESEET WATEEING PIACES BY CLYDE P. ROSS WASHINGTON GOVERNMENT PRINTING OFFICE 1923 ADDITIONAL COPIES OF THIS PUBLICATION MAT BE PROCURED FROM THE SUPERINTENDENT OF DOCUMENTS GOVERNMENT PRINTING OFFICE WASHINGTON, D. C. AT 50 CENTS PEE COPY PURCHASER AGREES NOT TO RESELL OR DISTRIBUTE THIS COPT FOR PROFIT. PUB. RES. 57, APPROVED MAT 11, 1822 CONTENTS. I Page. Preface, by O. E. Melnzer_____________ __ xr Introduction_ _ ___ __ _ 1 Location and extent of the region_____._________ _ J. Scope of the report- 1 Plan _________________________________ 1 General chapters _ __ ___ _ '. , 1 ' Route'descriptions and logs ___ __ _ 2 Chapter on watering places _ , 3 Maps_____________,_______,_______._____ 3 Acknowledgments ______________'- __________,______ 4 General features of the region___ _ ______ _ ., _ _ 4 Climate__,_______________________________ 4 History _____'_____________________________,_ 7 Industrial development___ ____ _ _ _ __ _ 12 Mining __________________________________ 12 Agriculture__-_______'.____________________ 13 Stock raising __ 15 Flora _____________________________________ 15 Fauna _________________________ ,_________ 16 Topography . _ ___ _, 17 Geology_____________ _ _ '. ___ 19 Bock formations. _ _ '. __ '_ ----,----- 20 Basal complex___________, _____ 1 L __. 20 Tertiary lavas ___________________ _____ 21 Tertiary sedimentary formations___T_____1___,r 23 Quaternary sedimentary formations _'__ _ r- 24 > Quaternary basalt ______________._________ 27 Structure _______________________ ______ 27 Geologic history _____ _____________ _ _____ 28 Early pre-Cambrian time______________________ . -
Sinuous Ridges in Chukhung Crater, Tempe Terra, Mars: Implications for Fluvial, Glacial, and Glaciofluvial Activity Frances E.G
Sinuous ridges in Chukhung crater, Tempe Terra, Mars: Implications for fluvial, glacial, and glaciofluvial activity Frances E.G. Butcher, Matthew Balme, Susan Conway, Colman Gallagher, Neil Arnold, Robert Storrar, Stephen Lewis, Axel Hagermann, Joel Davis To cite this version: Frances E.G. Butcher, Matthew Balme, Susan Conway, Colman Gallagher, Neil Arnold, et al.. Sinuous ridges in Chukhung crater, Tempe Terra, Mars: Implications for fluvial, glacial, and glaciofluvial activity. Icarus, Elsevier, 2021, 10.1016/j.icarus.2020.114131. hal-02958862 HAL Id: hal-02958862 https://hal.archives-ouvertes.fr/hal-02958862 Submitted on 6 Oct 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. 1 Sinuous Ridges in Chukhung Crater, Tempe Terra, Mars: 2 Implications for Fluvial, Glacial, and Glaciofluvial Activity. 3 Frances E. G. Butcher1,2, Matthew R. Balme1, Susan J. Conway3, Colman Gallagher4,5, Neil 4 S. Arnold6, Robert D. Storrar7, Stephen R. Lewis1, Axel Hagermann8, Joel M. Davis9. 5 1. School of Physical Sciences, The Open University, Walton Hall, Milton Keynes, MK7 6 6AA, UK. 7 2. Current address: Department of Geography, The University of Sheffield, Sheffield, S10 8 2TN, UK ([email protected]). -
Replace This Sentence with the Title of Your Abstract
MARS GLOBAL GEOLOGIC MAPPING: ABOUT HALF WAY DONE. K.L. Tanaka1, J.M. Dohm2, R. Ir- win3, E.J. Kolb4, J.A. Skinner, Jr.1, and T.M. Hare1. 1U.S. Geological Survey, Flagstaff, AZ, [email protected], 2U. Arizona, Tucson, AZ, 3Smithsonian Inst., Washington, DC, 4Google, Inc., CA. Introduction: We are in the third year of a five-year face appearance and apparent burial of underlying ma- effort to map the geology of Mars using mainly Mars terials in MOLA altimetry and THEMIS infrared and Global Surveyor, Mars Express, and Mars Odyssey imag- visible image data sets. It appears to be tens of meters ing and altimetry datasets. Previously, we have reported thick, similar in thickness of the pedestals underlying on details of project management, mapping datasets (local pedestal craters in the same region [4-5]. Thus, the unit and regional), initial and anticipated mapping approaches, appears to have retreated from a former extent. Prelimi- and tactics of map unit delineation and description [1-2]. nary analysis of crater counts and stratigraphic relations For example, we have seen how the multiple types and suggests that the unit is long-lived, likely emplaced huge quantity of image data as well as more accurate and over multiple episodes. These and other observations detailed altimetry data now available allow for broader and interpretations are the topic of a paper in prepara- and deeper geologic perspectives, based largely on im- tion by Skinner and Tanaka, to be submitted in summer proved landform perception, characterization, and analy- of 2009. sis. Here, we describe mapping and unit delineation re- Remaining work: Mapping tasks that remain in- sults thus far, a new unit identified in the northern plains, clude: (1) delineating and describing Noachian and and remaining steps to complete the map. -
FACT SHEET of Environmental Quality
SEPTEMBER 2013 Arizona Department FACT SHEET of Environmental Quality Janice K. Brewer, Governor • Henry R. Darwin, Director Publication Number: FS 13-11 Ambient Groundwater Quality of the Upper Hassayampa Basin: A 2003-2009 Baseline Study – June 2013 Introduction A baseline groundwater quality study of the Upper Hassayampa basin was con- ducted from 2003 to 2009 by the Arizona Department of Environmental Quality (ADEQ) Ambient Groundwater Monitor- ing Program. ADEQ carried out this task pursuant to Arizona Revised Statutes §49-225 that mandates ongoing moni- toring of waters of the state including its aquifers. This fact sheet is a synopsis of the ADEQ Open File Report 13-03.1 The Upper Hassayampa groundwater basin covers approximately 787 square miles within Maricopa and Yavapai counties and is located about 60 miles Map 1 – Sample sites in the northwest of Phoenix (Map 1). The basin Upper Hassayampa basin is characterized by mid-elevation moun- are color-coded according to their water quality status: No tains and had an estimated population Water Quality Exceedences, 2 of 10,479 in 2000. The largest popula- Secondary MCLs Exceedences, Primary MCL Exceedances, and Primary and Secondary MCL Exceedances. (Map by Jean Ann Rodine) tion center is the Town of Wickenburg. tions range from approximately 7,000 Other communities include Congress feet above mean sea level (amsl) in the and Groom Creek. Low-intensity livestock Bradshaw Mountains to 1,900 feet amsl grazing is the predominant land use and along the Hassayampa River about five most ranches have limited acreages of ir- miles south of Wickenburg. The basin is rigated pasture to raise additional animal comprised of federal land managed by feed. -
North Polar Region of Mars: Advances in Stratigraphy, Structure, and Erosional Modification
Icarus 196 (2008) 318–358 www.elsevier.com/locate/icarus North polar region of Mars: Advances in stratigraphy, structure, and erosional modification Kenneth L. Tanaka a,∗, J. Alexis P. Rodriguez b, James A. Skinner Jr. a,MaryC.Bourkeb, Corey M. Fortezzo a,c, Kenneth E. Herkenhoff a, Eric J. Kolb d, Chris H. Okubo e a US Geological Survey, Flagstaff, AZ 86001, USA b Planetary Science Institute, Tucson, AZ 85719, USA c Northern Arizona University, Flagstaff, AZ 86011, USA d Google, Inc., Mountain View, CA 94043, USA e Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA Received 5 June 2007; revised 24 January 2008 Available online 29 February 2008 Abstract We have remapped the geology of the north polar plateau on Mars, Planum Boreum, and the surrounding plains of Vastitas Borealis using altimetry and image data along with thematic maps resulting from observations made by the Mars Global Surveyor, Mars Odyssey, Mars Express, and Mars Reconnaissance Orbiter spacecraft. New and revised geographic and geologic terminologies assist with effectively discussing the various features of this region. We identify 7 geologic units making up Planum Boreum and at least 3 for the circumpolar plains, which collectively span the entire Amazonian Period. The Planum Boreum units resolve at least 6 distinct depositional and 5 erosional episodes. The first major stage of activity includes the Early Amazonian (∼3 to 1 Ga) deposition (and subsequent erosion) of the thick (locally exceeding 1000 m) and evenly- layered Rupes Tenuis unit (ABrt), which ultimately formed approximately half of the base of Planum Boreum. As previously suggested, this unit may be sourced by materials derived from the nearby Scandia region, and we interpret that it may correlate with the deposits that regionally underlie pedestal craters in the surrounding lowland plains. -
Mammal Footprints from the Miocene-Pliocene Ogallala
Mammalfootprints from the Miocene-Pliocene Ogallala Formation, easternNew Mexico by ThomasE. Williamsonand SpencerG. Lucas, New Mexico Museum of Natural History and Science,1801 Mountain Road NW Albuquerque, New Mexico 87104-7375 Abstract well-develooed mudcracks. The track- ways are diveloped on the mudstone Mammal trackways preserved in the drape but are preserved as infillings at the Miocene-Pliocene Ogallala Formation of base of the overlying conglomerate (Figs. eastern New Mexico represent the first 2-4). Most tracks are preserved on the report of mammal fossils-from this unit in underside of a single, thick conglomerate New Mexico. These trackwavs are Dre- block (Fig. 3). A few isolated mammal served as infillings in a conglomerate near the base of the Ogallala Formation. At least prints were also observed on the under- four mammalian ichnotaxa are represented, side of adjacent blocks.he depth of the including a single trackway of a large camel infillings suggest that tracks were made in (Gambapessp. A), several prints of an uncer- a relatively soft substrate. Some prints are tain family of artiodactyl (Gambapessp B), a accompanied by marks indicating slip- single trackway of a large feloid carnivoran page on a slick, wet substrate (Fig. 5C). (Bestiopeda sp.), and several indistinct im- Infillings of mudcracks and narrow, cylin- pressions, probably representing more than drical burrows and raindrop impressions one trackway of a small canid carnivoran are Dreserved over some areas of the (Chelipus sp ). The footprints are preserved in a channel-margin facies of an Ogallala tracliway slab. Mammal trackways repre- braided stream. sent at least four ichnotaxa. -
MARS ICE and POLAR PROCESSES 6:00 P.M
49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) sess638.pdf Thursday, March 22, 2018 [R638] POSTER SESSION II: MARS ICE AND POLAR PROCESSES 6:00 p.m. Town Center Exhibit Area Becerra P. Sori M. M. Thomas N. POSTER LOCATION #616 The Exposed Stratigraphy of the Martian South Polar Layered Deposits [#2445] A high-resolution quantitative study of the correlation and periodicities of the stratigraphic exposures in the South Polar Layered Deposits of Mars. Plaut J. J. Bellutta D. Gim Y. POSTER LOCATION #617 New Insights into the Internal Structure of the Martian Polar Plateaus from MARSIS 3D Mapping [#2252] We provide interpretation of new three-dimensional radar sounding image compilations of MARSIS data for both polar regions. Buhler P. B. Dickson J. Ehlmann B. L. Ingersoll A. P. Byrne S. et al. POSTER LOCATION #618 Prospects for Measuring Vertical Change on the Martian Residual South Polar Cap Using HiRISE Digital Elevation Models [#2908] We evaluate the prospect of using the difference between HiRISE DEMs taken at different times over the martian south polar cap to measure vertical change. Landis M. E. Byrne S. Dundas C. M. Herkenhoff K. E. Whitten J. L. et al. POSTER LOCATION #619 Surface Ages of the South Polar Layered Deposits, Mars [#1605] We present revised surface ages for the two geologic units of the South Polar Layered Deposits, Mars, based on crater counts using Context Camera (CTX) images. Gim Y. Bellutta D. Plaut J. POSTER LOCATION #620 Construction of MARSIS 3D Radar Maps of the Martian Polar Regions [#1793] We present 3D radar maps of the martian polar regions. -
The Meridiani Face on Mars
The Meridiani Face on Mars Greg Orme* School of Arts and Science, University of Queensland, Brisbane, Australia *Corresponding author: Greg Orme, School of Arts and Science, Undergraduate Science Student, University of Queensland, Brisbane, Australia, Tel: 07-33656195; E-mail: [email protected] Received: September 11, 2016; Accepted: November 25, 2016; Published: December 25, 2016 Abstract The Meridian Face has some similar features to the Cydonia and Crowned Faces such as having a crown. It is similar to the Nefertiti formation in that it seems to be made of dark soil, dunes in this case. Some dark dune fields can migrate large distances in Meridiani Planum, others remain confined in larger craters perhaps by shielding them from the wind. This can allow for the formation to be very old and remain intact. The similarity between the Crowned Face in the King’s Valley Libya Montes and the Meridiani Face was originally shown with an overall. The implicit hypothesis was that a new overlay would match the two faces even more closely, this has been borne out with the Crowned Face HiRise image and the Meridiani Face CTX image. Keywords: Meridiani planum; Barchan dune; Aeolian process; pareidolia; Dune migration Introduction The Meridiani Face was discovered around early June 2007 by a Mars researcher Terry James, (FIG. 1). The null hypothesis is that this is a random dune formation, an example of people’s innate ability to see faces [1]. It is proposed that this is falsified by the shape of these dunes, to be artificial they would have had to be moved to their current positions. -
Volcanism on Mars
Author's personal copy Chapter 41 Volcanism on Mars James R. Zimbelman Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC, USA William Brent Garry and Jacob Elvin Bleacher Sciences and Exploration Directorate, Code 600, NASA Goddard Space Flight Center, Greenbelt, MD, USA David A. Crown Planetary Science Institute, Tucson, AZ, USA Chapter Outline 1. Introduction 717 7. Volcanic Plains 724 2. Background 718 8. Medusae Fossae Formation 725 3. Large Central Volcanoes 720 9. Compositional Constraints 726 4. Paterae and Tholi 721 10. Volcanic History of Mars 727 5. Hellas Highland Volcanoes 722 11. Future Studies 728 6. Small Constructs 723 Further Reading 728 GLOSSARY shield volcano A broad volcanic construct consisting of a multitude of individual lava flows. Flank slopes are typically w5, or less AMAZONIAN The youngest geologic time period on Mars identi- than half as steep as the flanks on a typical composite volcano. fied through geologic mapping of superposition relations and the SNC meteorites A group of igneous meteorites that originated on areal density of impact craters. Mars, as indicated by a relatively young age for most of these caldera An irregular collapse feature formed over the evacuated meteorites, but most importantly because gases trapped within magma chamber within a volcano, which includes the potential glassy parts of the meteorite are identical to the atmosphere of for a significant role for explosive volcanism. Mars. The abbreviation is derived from the names of the three central volcano Edifice created by the emplacement of volcanic meteorites that define major subdivisions identified within the materials from a centralized source vent rather than from along a group: S, Shergotty; N, Nakhla; C, Chassigny. -
71St Annual Meeting Society of Vertebrate Paleontology Paris Las Vegas Las Vegas, Nevada, USA November 2 – 5, 2011 SESSION CONCURRENT SESSION CONCURRENT
ISSN 1937-2809 online Journal of Supplement to the November 2011 Vertebrate Paleontology Vertebrate Society of Vertebrate Paleontology Society of Vertebrate 71st Annual Meeting Paleontology Society of Vertebrate Las Vegas Paris Nevada, USA Las Vegas, November 2 – 5, 2011 Program and Abstracts Society of Vertebrate Paleontology 71st Annual Meeting Program and Abstracts COMMITTEE MEETING ROOM POSTER SESSION/ CONCURRENT CONCURRENT SESSION EXHIBITS SESSION COMMITTEE MEETING ROOMS AUCTION EVENT REGISTRATION, CONCURRENT MERCHANDISE SESSION LOUNGE, EDUCATION & OUTREACH SPEAKER READY COMMITTEE MEETING POSTER SESSION ROOM ROOM SOCIETY OF VERTEBRATE PALEONTOLOGY ABSTRACTS OF PAPERS SEVENTY-FIRST ANNUAL MEETING PARIS LAS VEGAS HOTEL LAS VEGAS, NV, USA NOVEMBER 2–5, 2011 HOST COMMITTEE Stephen Rowland, Co-Chair; Aubrey Bonde, Co-Chair; Joshua Bonde; David Elliott; Lee Hall; Jerry Harris; Andrew Milner; Eric Roberts EXECUTIVE COMMITTEE Philip Currie, President; Blaire Van Valkenburgh, Past President; Catherine Forster, Vice President; Christopher Bell, Secretary; Ted Vlamis, Treasurer; Julia Clarke, Member at Large; Kristina Curry Rogers, Member at Large; Lars Werdelin, Member at Large SYMPOSIUM CONVENORS Roger B.J. Benson, Richard J. Butler, Nadia B. Fröbisch, Hans C.E. Larsson, Mark A. Loewen, Philip D. Mannion, Jim I. Mead, Eric M. Roberts, Scott D. Sampson, Eric D. Scott, Kathleen Springer PROGRAM COMMITTEE Jonathan Bloch, Co-Chair; Anjali Goswami, Co-Chair; Jason Anderson; Paul Barrett; Brian Beatty; Kerin Claeson; Kristina Curry Rogers; Ted Daeschler; David Evans; David Fox; Nadia B. Fröbisch; Christian Kammerer; Johannes Müller; Emily Rayfield; William Sanders; Bruce Shockey; Mary Silcox; Michelle Stocker; Rebecca Terry November 2011—PROGRAM AND ABSTRACTS 1 Members and Friends of the Society of Vertebrate Paleontology, The Host Committee cordially welcomes you to the 71st Annual Meeting of the Society of Vertebrate Paleontology in Las Vegas. -
Sinuous Ridges in Chukhung Crater, Tempe Terra, Mars: Implications for Fluvial, Glacial, and Glaciofluvial Activity
This is a repository copy of Sinuous ridges in Chukhung crater, Tempe Terra, Mars: Implications for fluvial, glacial, and glaciofluvial activity. White Rose Research Online URL for this paper: http://eprints.whiterose.ac.uk/166644/ Version: Published Version Article: Butcher, F.E.G. orcid.org/0000-0002-5392-7286, Balme, M.R., Conway, S.J. et al. (6 more authors) (2021) Sinuous ridges in Chukhung crater, Tempe Terra, Mars: Implications for fluvial, glacial, and glaciofluvial activity. Icarus, 357. 114131. ISSN 0019-1035 https://doi.org/10.1016/j.icarus.2020.114131 Reuse This article is distributed under the terms of the Creative Commons Attribution (CC BY) licence. This licence allows you to distribute, remix, tweak, and build upon the work, even commercially, as long as you credit the authors for the original work. More information and the full terms of the licence here: https://creativecommons.org/licenses/ Takedown If you consider content in White Rose Research Online to be in breach of UK law, please notify us by emailing [email protected] including the URL of the record and the reason for the withdrawal request. [email protected] https://eprints.whiterose.ac.uk/ Journal Pre-proof Sinuous ridges in Chukhung crater, Tempe Terra, Mars: Implications for fluvial, glacial, and glaciofluvial activity Frances E.G. Butcher, Matthew R. Balme, Susan J. Conway, Colman Gallagher, Neil S. Arnold, Robert D. Storrar, Stephen R. Lewis, Axel Hagermann, Joel M. Davis PII: S0019-1035(20)30473-5 DOI: https://doi.org/10.1016/j.icarus.2020.114131 Reference: YICAR 114131 To appear in: Icarus Received date: 2 June 2020 Revised date: 19 August 2020 Accepted date: 28 September 2020 Please cite this article as: F.E.G. -
Durangoko Azoka & Durango Da Azoka
egitaraua Durangoko azoka & Durango da azoka Durango uriaren hegaletik Mañarierreka bideratzen da Kantauri itsasoaren bila. Erreka-bazterrean, urtero, 1965az geroztik, gizaki-tantekin osatutako Durangoko azoka izeneko ur-putzua sortzen izan da. Baina… nahiz eta urtero ur berria izan putzuak, lau hamarkada luze igaro ondoren tanta, beste tanta batzuekin bilduz, putzu izateari utzi eta erreka izatearen beharra ikusi zuten. Putzua Kulturerreka bihurtzea. Errekaondoko bidezidorrean zehar, abenduko euri zaparradako tangadak bilduz, euskal kulturaren uholdea sortu eta bideratu. Landakotik Larizdorre kalera kokatzen diren azoka, saguganbara, ahotsenea, irudienea, szenatokia eta beste izen batzuetako ur-putzuak lotuz Errekaondoko kultur bidezidorra burutu. Tabirako Uriberri guztira AZOKA zabalduz. Durangoko azoka & Durango da azoka. Aurkibidea 04 Durangoko mapa 06 Landako erakustazoka 08 Artisau Azoka 09 Abenduaren 5ean 13 Abenduaren 6an 17 Abenduaren 7an 21 Abenduaren 8an Erretentxu K. Kurutziaga Kalea Matxinestarta Kalea Ibaizabal Auzunea Pablo Pedro Astarloa Kalea Murueta Torre A. Murueta Torre Komentukalea Kalea Andra Mari Kalea 1 2 3 Antso Estegiz Zumardia Aldapa Azoka Kabi@ Areto Nagusia Arandoño Torre K. Kalebarria K. Azoka K. Goienkalea Kalea Monago K. P Parkinga Hiribidea Montevideo Artisau Azoka Kanpatorrosteta K. Artekalea Kalea Uribarri Kalea Barrenkalea K. Oiz Kalea 4 5 6 7 Lariz Torre K. Saguganbara Plateruena Ahotsenea Irudienea Zeharkalea K. Andra Mari K. Oiz Kalea Oiz Zumalakarregi K. Zumalakarregi K. 8 Szenatokia Arkotxa K. Arkotxa Turismo Ermodo Kalea Bulegoa Bus Geltokia Ezkurdi Plaza Arte eta Historia Museoa Juan Antonio Abasolo K Geltoki Zaharra Argazki Erakusketa “Noctis Labyrinthus” Josemiel Barandiaran K, Tronperri Kalea Galtzareta K. Tren Landako Hiribidea Geltokia Bruno Mauricio Zabala K. Fray Juan de Zumarraga K. 4 2013ko abenduaren 5etik 8ra Erretentxu K.